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Loop Quantum Gravity

(i).. The computation of the physical spectra of geometrical quantities such as area and volume, which yields quantitative predictions on Planck-scale physics. (ii).. A derivation of the Bekenstein-Hawking black hole entropy formula. (iii).. An intriguing physical picture of the microstructure of qu...

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Detalles Bibliográficos
Autor principal: Rovelli, Carlo
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer International Publishing 1998
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5567241/
https://www.ncbi.nlm.nih.gov/pubmed/28937180
http://dx.doi.org/10.12942/lrr-1998-1
Descripción
Sumario:(i).. The computation of the physical spectra of geometrical quantities such as area and volume, which yields quantitative predictions on Planck-scale physics. (ii).. A derivation of the Bekenstein-Hawking black hole entropy formula. (iii).. An intriguing physical picture of the microstructure of quantum physical space, characterized by a polymer-like Planck scale discreteness. This discreteness emerges naturally from the quantum theory and provides a mathematically well-defined realization of Wheeler’s intuition of a spacetime “foam”. Long standing open problems within the approach (lack of a scalar product, over-completeness of the loop basis, implementation of reality conditions) have been fully solved. The weak part of the approach is the treatment of the dynamics: at present there exist several proposals, which are intensely debated. Here, I provide a general overview of ideas, techniques, results and open problems of this candidate theory of quantum gravity, and a guide to the relevant literature.